Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume....
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Format: | Journal article |
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2005
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author | Balasubramanian, V Berglund, P Conlon, J Quevedo, F |
author_facet | Balasubramanian, V Berglund, P Conlon, J Quevedo, F |
author_sort | Balasubramanian, V |
collection | OXFORD |
description | We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of the string scale to the 4d Planck scale is hierarchically small but flux dependent. The inclusion of alpha' corrections plays a crucial role in the structure of the potential. We illustrate these ideas through explicit computations for a particular Calabi-Yau manifold. |
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format | Journal article |
id | oxford-uuid:15998a41-abdd-4f61-a550-9dffc6ebea2e |
institution | University of Oxford |
last_indexed | 2024-03-06T19:07:21Z |
publishDate | 2005 |
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spelling | oxford-uuid:15998a41-abdd-4f61-a550-9dffc6ebea2e2022-03-26T10:26:25ZSystematics of Moduli Stabilisation in Calabi-Yau Flux CompactificationsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:15998a41-abdd-4f61-a550-9dffc6ebea2eSymplectic Elements at Oxford2005Balasubramanian, VBerglund, PConlon, JQuevedo, FWe study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of the string scale to the 4d Planck scale is hierarchically small but flux dependent. The inclusion of alpha' corrections plays a crucial role in the structure of the potential. We illustrate these ideas through explicit computations for a particular Calabi-Yau manifold. |
spellingShingle | Balasubramanian, V Berglund, P Conlon, J Quevedo, F Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title | Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title_full | Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title_fullStr | Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title_full_unstemmed | Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title_short | Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications |
title_sort | systematics of moduli stabilisation in calabi yau flux compactifications |
work_keys_str_mv | AT balasubramanianv systematicsofmodulistabilisationincalabiyaufluxcompactifications AT berglundp systematicsofmodulistabilisationincalabiyaufluxcompactifications AT conlonj systematicsofmodulistabilisationincalabiyaufluxcompactifications AT quevedof systematicsofmodulistabilisationincalabiyaufluxcompactifications |